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Table A.1

Restframe UV-to-FIR photometry sets for our sample (AB magnitudes up to the IRAC bands included, then in mJy) with 1σ uncertainties.

Observing band C0 h7 HLS115 nn4 MACS0451a

B 22.300 ± 0.104 23.298 ± 0.131 22.968 ± 0.048 <26.60 20.838 ± 0.020
g 20.606 ± 0.045
V 20.425 ± 0.020
F602W 20.347 ± 0.020
R 21.994 ± 0.050 <26.28
r 20.175 ± 0.050
F702W 21.154 ± 0.083 21.896 ± 0.050
i 20.299 ± 0.076
Ic 20.148 ± 0.020
F814W 20.802 ± 0.078 21.602 ± 0.027 21.450 ± 0.060 20.062 ± 0.020
z 21.360 ± 0.053 21.144 ± 0.072 24.70 ± 0.21
J/ISAAC 20.104 ± 0.029 20.278 ± 0.049 22.98 ± 0.06
F110W 19.643 ± 0.031 19.675 ± 0.020
F140W 19.181 ± 0.020
F160W 19.118 ± 0.030
H/ISAAC 19.775 ± 0.040 19.928 ± 0.052 22.33 ± 0.06
Ks 18.643 ± 0.091 19.470 ± 0.036 19.285 ± 0.030 21.45 ± 0.04
IRAC 3.6 μm 17.925 ± 0.061 18.635 ± 0.027 18.885 ± 0.029 20.53 ± 0.04 18.913 ± 0.020
IRAC 4.5 μm 17.693 ± 0.067 18.441 ± 0.038 18.677 ± 0.031 20.15 ± 0.04 18.898 ± 0.020

MIPS 24 μm (mJy) 0.945 ± 0.060 0.341 ± 0.060 0.69 ± 0.06 <0.20
PACS 100 μm (mJy) 7.73 ± 0.38 8.37 ± 0.37 19.96 ± 0.37 8.58 ± 0.37 9.86 ± 0.60
PACS 160 μm (mJy) 31.26 ± 0.95 24.61 ± 0.95 41.48 ± 0.96 25.26 ± 0.95 17.67 ± 0.95
SPIRE 250 μm (mJy) 46.68 ± 1.68 40.16 ± 1.33 53.59 ± 1.75 45.30 ± 1.87 17.61 ± 3.18
SPIRE 350 μm (mJy) 39.88 ± 1.68 27.36 ± 1.48 37.84 ± 1.64 38.04 ± 2.19 11.27 ± 3.29
SPIRE 500 μm (mJy) 21.47 ± 1.13 12.01 ± 1.29 18.64 ± 1.22 17.74 ± 1.50   5.24 ± 2.69
SCUBA2 850 μm (mJy) 5.39 ± 0.23 3.26 ± 0.70 3.02 ± 0.65

Notes. B and R bands correspond to CFHT/12k for A68, whereas B, V, and Ic in the case of MACS0451 correspond to Subaru’s SuprimeCam. Ks photometry comes from UKIRT, z is from VLT/FORS2, and g,   r,   i from SDSS.

(a)

For MACS0451 we present the FIR photometry of the northern part, and the stellar emission of the full arc. We have established that the northern part accounts for ~40% of the total emission in the visible.

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